CHAPTER 4. CONFORMAL INVARIANCE 58in which 8β g µν = α ′ (R µν + 2∇ µ ∇ ν Φ − 1 4 H µκσH κσν)+ O ( α ′2) , (4.20)(βµν B = α ′ − 1 )2 ∇κ H κµν + ∇ κ ΦH κµν + O ( α ′2) , (4.21)( D − 26β Φ = α ′ 6α ′ − 1 2 ∇2 Φ + ∇ κ Φ∇ κ Φ − 1 )24 H κµνH κµν + O ( α ′2) , (4.22)where we usedH κµν = ∂ κ B µν + ∂ µ B νκ + ∂ ν B κµ .These are the generalized Einstein equati<strong>on</strong>s for the fields under c<strong>on</strong>siderati<strong>on</strong>. Notethat the expansi<strong>on</strong> in α ′ is <strong>on</strong>ly valid if the typical length scale <str<strong>on</strong>g>of</str<strong>on</strong>g> space-time (usuallyexpressed in terms <str<strong>on</strong>g>of</str<strong>on</strong>g> the Ricci scalar) is much larger than α ′ , or equivalently if spacetimeis <strong>on</strong>ly slightly curved at the string length scale (recall that l 2 s = 2α ′ ). The acti<strong>on</strong>for the scalar field, being <strong>on</strong>e order higher in α ′ , can be c<strong>on</strong>sidered as a first orderperturbative correcti<strong>on</strong>.Demanding that Weyl invariance is still respected implies that all above menti<strong>on</strong>edβ-functi<strong>on</strong>s should vanish, in turn demanding that the world sheet theory is describedby a c<strong>on</strong>formal field theory, i.e. a scale invariant theory. It should be noted that whenβ g = β B = 0, we are left withT α α = − 1 2 βΦ R (2) , (4.23)which as we saw is exactly the c<strong>on</strong>formal anomaly that arises when <strong>on</strong>e quantizes atwo-dimensi<strong>on</strong>al c<strong>on</strong>formal field theory. Hence, when β g = β B = 0, Eq. 4.18 describesa c<strong>on</strong>formal field theory with central charge equaling β Φ . 9 Since β Φ should also vanish,we are left with an anomaly free c<strong>on</strong>formal field theory.Furthermore, it is worth pointing out that when all above β-functi<strong>on</strong>s are set to zero,what remains are sec<strong>on</strong>d order differential equati<strong>on</strong>s for the background fields. As itturns out, these can be regrouped into <strong>on</strong>e single acti<strong>on</strong>,S = 12κ 2 0∫d D X √ −Ge −2φ [R + 4∇ µ Φ∇ µ Φ − 1 12 H µνλH µνλ2 (D − 26)−3α ′ + O ( α ′)] , (4.24)in which κ 0 represents a c<strong>on</strong>stant with no physical significance, as it can be absorbed ina redefiniti<strong>on</strong> <str<strong>on</strong>g>of</str<strong>on</strong>g> Φ. Varying this acti<strong>on</strong> with respect to the background fields results insaid differential equati<strong>on</strong>s. Remark that from this, if <strong>on</strong>e splits Φ into its expectati<strong>on</strong>value Φ 0 and the deviati<strong>on</strong> there<str<strong>on</strong>g>of</str<strong>on</strong>g>, Φ −→ Φ 0 + Φ, <strong>on</strong>e can identify g s = e Φ 0. In otherwords, the expectati<strong>on</strong> value <str<strong>on</strong>g>of</str<strong>on</strong>g> the scalar field Φ defines the string coupling c<strong>on</strong>stant.If so wanted, <strong>on</strong>e could redefine the metric G µν −→ ˜G µν by multiplying with a suitable8 Readers curious as to the details <str<strong>on</strong>g>of</str<strong>on</strong>g> the derivati<strong>on</strong>s <str<strong>on</strong>g>of</str<strong>on</strong>g> these β-functi<strong>on</strong>s are referred to §2.1.3 in [5].9 It can be shown that when β g = β B = 0, β Φ is c<strong>on</strong>stant.
CHAPTER 4. CONFORMAL INVARIANCE 59power <str<strong>on</strong>g>of</str<strong>on</strong>g> e Φ in order to bring the gravitati<strong>on</strong>al part <str<strong>on</strong>g>of</str<strong>on</strong>g> the acti<strong>on</strong> to the standard Hilbertform 1 ∫2κ d X√D − ˜GR, allowing <strong>on</strong>e to identifyκ ≡ κ 0 e Φ 0= √ 8πG N , (4.25)with G N Newt<strong>on</strong>’s gravitati<strong>on</strong>al c<strong>on</strong>stant. Details can be found in §3.7 in [18] or §2.7in [12].4.3 SummaryThe few preceding pages attempted to highlight some <str<strong>on</strong>g>of</str<strong>on</strong>g> the essential characteristics <str<strong>on</strong>g>of</str<strong>on</strong>g>a c<strong>on</strong>formal field theory. Then a short review was given <str<strong>on</strong>g>of</str<strong>on</strong>g> the problems associated withthe generalizati<strong>on</strong> <str<strong>on</strong>g>of</str<strong>on</strong>g> (bos<strong>on</strong>ic) string theory from flat space-time to curved space-times,further including the Kalb-Ram<strong>on</strong>d and scalar Φ background fields, and it was shownthat the resoluti<strong>on</strong> <str<strong>on</strong>g>of</str<strong>on</strong>g> these problems demanded that the world sheet theory be describedby a c<strong>on</strong>formal field theory. It was further brought forward that the expectati<strong>on</strong> value<str<strong>on</strong>g>of</str<strong>on</strong>g> the Φ field in fact determines the string coupling g s .